The possible protogalactic role of eddies in a turbulent early universe

Details The possible protogalactic role of eddies in a turbulent early universe The possible protogalactic role of eddies in a turbulent early universe

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.115..257b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 115, no. 2, Oct. 1985, p. 257-265. DOE-sponsored research.

Astronomy and Astrophysics

Astrophysics

3

Astronomical Models, Galactic Evolution, Gravitational Collapse, Missing Mass (Astrophysics), Turbulence, Vortices, Cosmology, Mass Distribution, Rotating Matter, Universe

Scientific paper

It is shown that eddies, present in a turbulent early universe, can form
excellent galaxies upon collapse of the eddies and a small amount of
viscous evolution. The resulting model galaxies display realistically
flat rotation curves as well as exponential-like luminosity profiles.
The dark mass is allowed to be non-baryonic in this model.

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